Results 121 to 130 of about 21,959 (162)

Galaxy Tomography with the Gravitational Wave Background from Supermassive Black Hole Binaries

Chen Y.
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High energy neutrino astronomy

Nature, 1978
The possibility of doing point source neutrino astronomy is discussed. Probable sources include galactic nuclei, Seyferts, quasars, radio galaxies, pulsars and supernovae.
David Eichler, David N. Schramm
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High-energy Gamma-ray Astronomy

Nature, 1970
Gamma-ray astronomy above 10 MeV is difficult from the experimental point of view, but promising data are beginning to appear, as this survey progress report shows.
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The high energy astronomy observatories

13th Annual Meeting and Technical Display Incorporating the Forum on the Future of Air Transportation, 1977
The forthcoming NASA project of orbiting High Energy Astronomy Observatories (HEAO's) designed to probe the universe by tracing celestial radiations and particles is outlined. Solutions to engineering problems concerning HEAO's which are integrated, yet built to function independently are discussed, including the onboard digital processor, mirror ...
A. NEIGHBORS, R. DOOLITTLE, R. HALPERS
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High-energy neutrino astronomy

La Rivista del Nuovo Cimento, 2010
The field of astroparticle physics entered in a flourishing period thanks to the operation of several experiments that lead to the discovery and even identification of about hundred cosmic TeV gamma-ray sources and measurement of the Ultra-High-Energy Cosmic-Ray flux.
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Very high energy gamma ray astronomy

AIP Conference Proceedings, 1988
Abstract Current interest in gamma-astronomy at energies above 100 GeV comes from the identification of Cygnus X-3 and other X-ray binaries as sources. In addition there are reports of emission from radio pulsars and a variety of other objects. The statistical significance of many of the observations is not high and many reported effects await ...
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Ultra High Energy Astronomy

1989
Techniques of Ultra High Energy astronomy are reviewed in this lecture. Sensitivity of experiments currently underway or planned for the near future is discussed. Recent results from the CYGNUS experiment with regard to steady emission from sources such as Cygnus X-3 and Herculus X-l are compared with those from other experiments.
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High-Energy Gamma-Ray Astronomy

IEEE Transactions on Nuclear Science, 1963
The search for gamma radiation with energy greater than 50 Mev from extraterrestrial sources has resulted in some of the most interesting and most difficult balloon and spacecraft experiments. The present status of this search is reviewed. The first attempt to detect this radiation from solar flares resulted in no increase of the counting rate above ...
G. G. Fazio, C. J. Cook, E. M. Hafner
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High Energy Astronomy Observatory Program

IFAC Proceedings Volumes, 1978
Abstract This paper describes the series of three orbiting high energy astronomy observatories that comprise the High Energy Astronomy Observatory (HEAO) program of the National Aeronautics and Space Administration (NASA). The basis and enthusiasm of the scientific community for this program is presented.
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High Energy Cosmic Ray Astronomy

Nuclear Physics B - Proceedings Supplements, 1996
A brief introduction to High Energy Cosmic Ray Astronomy is presented. This field covers a 17 decade energy range (2×10 4 – 10 20 ) eV. Recent discoveries done with gamma-ray detectors on-board satellites and ground-based Cherenkov devices are pushing for a fast development of new and innovative techniques, specially in the low energy region which ...
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